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In order to enable an iCal export link, your account needs to have a key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.

I have read and understood the above.

In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.

I have read and understood the above.

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Contribution
Oral presentation

Recent highlights of the MAGIC telescopes

Speakers

Primary authors

Abstract content

MAGIC (Major Atmospheric Gamma Imaging Cherenkov) is a
system of two imaging atmospheric Cherenkov telescopes located at the
Canary island of La Palma. The telescopes are performing observations
of gamma rays with energies between 50 GeV and tens of TeV. In 2014
MAGIC celebrated its 10th anniversary of scientific operations. In
this talk I will present the recent highlights of the observations
performed with the MAGIC telescopes. I will discuss the ultra-fast
variability of IC 310, challenging jet emission models in AGNs.
I will present the detection of the VHE gamma-ray emission from
two active galaxies located at redshift of ~0.94: gravitationally
lensed blazar B0218+357 and FSRQ PKS 1441+25. Finally, I will also
present the newest measurements of the VHE emission from Crab pulsar.